{
  "abstract": "We present our first result from an ongoing pulsar glitch monitoring campaign at the Canadian Hydrogen Intensity Mapping Experiment (CHIME), in which we analyzed the radio and X-ray emission surrounding four glitches in PSR~J2229+6114. Using daily CHIME observations, we detected a glitch in PSR~J2229+6114 in near-real time and triggered an X-ray follow-up with the Nuclear Spectroscopic Telescope Array (NuSTAR) two days after the glitch. We identified three additional glitch events in archival CHIME/Pulsar observations that coincided with an independent X-ray observing campaign with the Neutron star Interior Composition Explorer (NICER).. Our data show there is no measurable change in the source's X-ray and radio emission during the four glitch events, in stark contrast to the post-glitch activity in high-magnetic-field, rotation-powered pulsars (RPPs), which have been observed to exhibit magnetar-like X-ray outbursts immediately after large glitches. Those high-magnetic-field (high-$B$) RPPs are considered transitional objects between ordinary RPPs and magnetars, thereby leading to a unifying neutron star model in which the inferred dipolar surface magnetic field strength serves as a unifying parameter. However, such a model remains challenged, in part, by the lack of constraints near the low-$B$ end of the high-$B$ regime, and our result provides additional evidence that magnetar-like post-glitch activity is likely more common among high-$B$ RPPs.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2605.13011",
  "author_total": 14,
  "authors": [
    {
      "name": "Wenke Xia"
    },
    {
      "name": "Robert A. Main"
    },
    {
      "name": "Mason Ng"
    },
    {
      "name": "Victoria M. Kaspi"
    },
    {
      "name": "Jason W. Hessels"
    },
    {
      "name": "Alyssa Cassity"
    },
    {
      "name": "Abigail K. Denney"
    },
    {
      "name": "Emmanuel Fonseca"
    },
    {
      "name": "Deborah C. Good"
    },
    {
      "name": "Ajay Kumar"
    },
    {
      "name": "Lars Kunkel"
    },
    {
      "name": "Bradley W. Meyers"
    },
    {
      "name": "Aaron B. Pearlman"
    },
    {
      "name": "Ingrid Stairs"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/7k0zznn5fcw9c.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2605.13011",
  "fulltext_url": null,
  "id": "7k0zznn5fcw9c",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2605.13011",
  "language": null,
  "licence": "CC-BY-4.0",
  "licence_label": "CC BY 4.0",
  "licence_source": "article",
  "licence_url": "http://creativecommons.org/licenses/by/4.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.HE"
    ]
  ],
  "openalex": null,
  "pdf_url": "https://arxiv.org/pdf/2605.13011",
  "pmcid": null,
  "pmid": null,
  "published": "2026-09-01",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/7k0zznn5fcw9c.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:18:16Z",
      "native_id": "2605.13011",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2605.13011"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.HE",
      "subfield": "high-energy-astrophysics"
    }
  ],
  "title": "No Measurable Changes in Radio and X-ray Emission Surrounding Glitches in the Young Pulsar PSR J2229+6114",
  "title_text": "No Measurable Changes in Radio and X-ray Emission Surrounding Glitches in the Young Pulsar PSR J2229+6114",
  "type": "preprint",
  "updated_at": "2026-10-30T12:18:16Z",
  "url": "https://research.draconitic.com/paper/7k0zznn5fcw9c",
  "venue": "arXiv",
  "versions": [
    {
      "doi": "10.3847/1538-4357/ae9758",
      "pid": null,
      "relation": "published-as",
      "title": null,
      "venue": null
    }
  ]
}